Influence of Finite Collision Time on Energy Density in Relativistic Heavy Ion Collisions

Soren P. Sorensen; Zhao Weiqin

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 1993, Vol. 17> Issue(S1) : 89-93

Influence of Finite Collision Time on Energy Density in Relativistic Heavy Ion Collisions

Soren P. Sorensen ¹ ,
Zhao Weiqin ²

1 University of Tennessee, Knoxville, TN 37796, USA, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA;
2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China

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The space-time development of the energy density reached in relativistic heavy ion collisions is analyzed based on the Monte Carlo code ODEN. The results show that the actually reached energy density is considerably lower than Bjorken's estimation due to the finite collision time.

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Soren P. Sorensen and Zhao Weiqin. Influence of Finite Collision Time on Energy Density in Relativistic Heavy Ion Collisions[J]. Chinese Physics C, 1993, 17(S1): 89-93.

Soren P. Sorensen and Zhao Weiqin. Influence of Finite Collision Time on Energy Density in Relativistic Heavy Ion Collisions[J]. Chinese Physics C, 1993, 17(S1): 89-93. shu

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Received: 1992-11-13

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Partly supported by the National Natural Science Foundation of China and US Department of Energy.

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沈阳化工大学材料科学与工程学院沈阳 110142

Influence of Finite Collision Time on Energy Density in Relativistic Heavy Ion Collisions

Soren P. Sorensen ^1,
Zhao Weiqin ^2,

1 University of Tennessee, Knoxville, TN 37796, USA, Oak Ridge National Laboratory, Oak Ridge, TN 37831, USA;
2 Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, China

Received Date: 1992-11-13

Fund Project: Partly supported by the National Natural Science Foundation of China and US Department of Energy.

Abstract: The space-time development of the energy density reached in relativistic heavy ion collisions is analyzed based on the Monte Carlo code ODEN. The results show that the actually reached energy density is considerably lower than Bjorken's estimation due to the finite collision time.